AGASC ID 31983224

Info

Last Obs. 2023:051:11:20
magcatalog 9.42 ± 0.10
mag3 arcsec 9.47 ± 0.02
mag5 arcsec 9.47 ± 0.02
Nobs 32 (0 bad)
fok 99.0%
f3 arcsec 100.0%
f5 arcsec 100.0%

Timeline

Observation Info

OBSID Time Slot Row Col N Nmag est ok Nout fmag est ok fdr3 fdbox5 fmag est ok 3 ⟨ δ mag ⟩ 100s ⟨ mag ⟩ σmag Comments
8494 2006:350:13:11:39.686 7 298.2 -445.4 10536 10519 17 99.8% 100.0% 100.0% 99.8% 0.02 9.49 0.00 --
8002 2006:353:04:48:16.684 4 190.1 -443.2 14910 14893 17 99.9% 100.0% 100.0% 99.9% 0.03 9.50 0.00 --
8007 2006:353:22:09:03.821 5 87.5 -435.4 11078 11058 22 99.8% 100.0% 100.0% 99.8% 0.03 9.50 0.00 --
8496 2006:357:11:57:15.560 4 190.1 -443.2 10119 9600 17 99.8% 100.0% 100.0% 99.8% 0.02 9.50 0.00 --
8497 2006:359:01:35:19.124 5 87.5 -435.4 13743 13622 21 99.1% 100.0% 100.0% 99.1% 0.04 9.50 0.00 --
7997 2006:364:21:00:05.856 4 280.5 -367.2 22723 22384 28 98.5% 100.0% 100.0% 98.5% 0.03 9.48 0.00 --
8013 2007:004:19:42:33.222 5 -32.6 -424.2 23996 23950 45 99.8% 100.0% 100.0% 99.8% 0.03 9.46 0.00 --
8001 2007:092:03:45:37.538 7 -268.7 232.9 24054 23997 37 99.8% 100.0% 100.0% 99.7% 0.04 9.45 0.00 --
8017 2007:094:17:53:24.980 3 23.2 261.8 23310 23277 36 99.9% 100.0% 100.0% 99.8% 0.03 9.48 0.00 --
8018 2007:095:07:15:14.980 6 15.0 358.1 23985 23452 37 99.8% 100.0% 100.0% 99.8% 0.03 9.48 0.00 --
8123 2007:097:13:38:13.480 7 -273.4 333.8 24481 24345 49 99.4% 100.0% 100.0% 99.4% 0.03 9.45 0.00 --
8025 2007:102:11:55:27.181 6 103.2 463.3 24482 24451 39 99.9% 100.0% 100.0% 99.9% 0.02 9.47 0.00 --
8550 2007:108:18:48:03.261 3 31.4 165.7 12129 11613 25 99.8% 100.0% 100.0% 99.8% 0.03 9.48 0.00 --
8016 2007:109:20:05:13.981 3 31.4 165.7 11798 11770 29 99.8% 100.0% 100.0% 99.7% 0.03 9.47 0.00 --
54105 2012:345:21:33:35.517 3 419.6 -435.9 46 46 0 100.0% 100.0% 100.0% 100.0% 0.01 9.49 0.00 --
15225 2013:095:06:44:18.659 4 204.0 194.3 24925 23858 31 95.7% 100.0% 100.0% 95.7% 0.05 9.47 0.00 --
53730 2013:122:16:38:46.132 1 36.2 58.9 45 45 0 100.0% 100.0% 100.0% 100.0% 0.01 9.47 0.00 --
15230 2013:128:15:48:22.688 4 -248.4 55.3 24594 24040 29 97.8% 100.0% 100.0% 97.7% 0.03 9.45 0.00 --
53708 2013:130:14:55:01.206 1 -157.0 56.7 171 164 0 95.9% 100.0% 100.0% 95.9% 0.01 9.46 0.00 --
15232 2013:136:09:28:20.496 3 -442.1 56.0 24809 24535 35 98.9% 100.0% 100.0% 98.9% 0.06 9.47 0.00 --
15649 2013:154:05:15:10.118 3 -442.1 56.0 7605 7532 11 99.1% 100.0% 100.0% 99.0% 0.04 9.48 0.00 --
53659 2013:154:09:57:24.508 1 -442.1 56.0 46 45 0 100.0% 100.0% 100.0% 100.0% 0.01 9.48 0.00 --
15246 2013:295:18:15:20.138 6 -321.6 -463.0 24264 23777 29 98.0% 100.0% 100.0% 98.0% 0.05 9.44 0.00 --
15248 2013:317:01:16:12.306 4 -354.6 -248.0 24458 24303 27 99.4% 100.0% 100.0% 99.3% 0.05 9.45 0.00 --
53198 2013:334:06:53:31.955 0 -163.4 49.7 230 227 0 98.7% 100.0% 100.0% 98.7% 0.04 9.44 0.00 --
15260 2014:005:19:40:07.498 3 -38.3 153.4 11285 11122 4 98.6% 100.0% 100.0% 98.6% 0.07 9.48 0.00 --
16562 2014:008:03:22:23.230 3 -38.3 153.4 13726 13508 27 98.4% 100.0% 100.0% 98.4% 0.05 9.46 0.00 --
15262 2014:012:20:03:19.256 3 153.6 117.1 24846 24663 30 99.3% 100.0% 100.0% 99.3% 0.06 9.48 0.00 --
16562 2014:025:14:14:53.876 3 -38.3 153.4 13231 12931 22 97.7% 100.0% 100.0% 97.7% 0.07 9.46 0.00 --
15247 2014:077:01:59:15.464 6 222.7 430.7 24524 24308 22 99.1% 100.0% 100.0% 99.1% 0.06 9.47 0.00 --
52918 2014:077:16:25:46.087 5 222.7 430.7 45 45 0 100.0% 100.0% 100.0% 100.0% 0.01 9.47 0.00 --
44802 2023:051:11:20:06.000 5 165.8 163.4 1327 1311 1 98.8% 99.8% 100.0% 98.6% 0.13 9.56 0.00 --

  • sample: One sample of ACA image telemetry. This could be a real image readout or it could be a null 4x4 image when the ACA is not tracking. Be aware that the sample period is faster for null 4x4 images (1.025 sec) than for typical 6x6 or 8x8 tracked images (2.05 or 4.1 sec respectively).
  • Kalman samples: Subset of samples when ACA could be tracking stars (AOPCADMD == NPNT & AOACASEQ == KALM)
  • dr3: Subset of tracked Kalman samples with radial centroid residual < 3 arcsec. This corresponds to "high quality" readouts. This effectively includes the track subset (AOACFCT == TRAK) because readouts with no TRAK are assigned an infinite centroid residual.
  • dbox5: Subset of tracked Kalman samples with centroid residual within a 5 arcsec box. This corresponds to spatial filter used by the OBC for inclusion in Kalman filter. This effectively includes the track subset (AOACFCT == TRAK) because readouts with no TRAK are assigned an infinite centroid residual.
  • track: Subset of Kalman samples where the image is being tracked (AOACFCT == TRAK)
  • sat_pix: Subset of Kalman samples with saturated pixel flag OK (AOACISP == OK)
  • ion_rad: Subset of Kalman samples with ionizing radiation flag OK (AOACIIR == OK)
  • mag_est_ok: Subset of Kalman samples that have a magnitude estimate (track & ion_rad)
  • n_total: Total number of sample regardless of OBC PCAD status
  • n: Synonym for n_total
  • n_kalman: Number of Kalman samples
  • n_dr3: Number of dr3 samples.
  • n_dbox5: Number of dbox5 samples.
  • n_track: Number of track samples.
  • n_ok_3: Number of (track & sat_pix & ion_rad & dr3) samples
  • n_ok_5: Number of (track & sat_pix & ion_rad & dbox5) samples
  • n_mag_est_ok: Number of (track & ion_rad) samples
  • n_mag_est_ok_3: Number of (track & ion_rad & dr3) samples
  • n_mag_est_ok_5: Number of (track & ion_rad & dbox5) samples
  • f_dr3: Fraction of mag-est-ok samples with centroid residual < 3 arcsec((mag_est_ok & n_dr3)/n_mag_est_ok)
  • f_dbox5: Fraction of mag-est-ok samples with centroid within 5 arcsec box((mag_est_ok & n_dbox5)/n_mag_est_ok)
  • f_mag_est_ok: n_mag_est_ok_3/n_kalman. This is a measure of the fraction of time during an observation that a magnitude estimate is available.
  • f_mag_est_ok_3: n_mag_est_ok_3/n_kalman.
  • f_mag_est_ok_5: n_mag_est_ok_5/n_kalman.
  • f_ok: n_ok_5 / n_kalman. Same as f_ok_5
  • f_ok_3: n_ok_3 / n_kalman. This is a measure of the fraction of time during an observation that the Kalman filter is getting high-quality star centroids.
  • f_ok_5: n_ok_5 / n_kalman. This is a measure of the fraction of time during an observation that the Kalman filter is getting any star centroid at all. This includes measurements out to 5 arcsec box halfwidth, so potentially 7 arcsec radial offset.